Journal ArticleAstronomical Journal · June 2, 2025
We investigate the capability of the Nancy Grace Roman Space Telescope’s (Roman) Wide-Field Instrument G150 slitless grism to detect red, quiescent galaxies based on the current reference survey. We simulate dispersed images for Roman reference High-Latitu ...
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Journal ArticlePhysical review letters · January 2025
The Super-Kamiokande and T2K Collaborations present a joint measurement of neutrino oscillation parameters from their atmospheric and beam neutrino data. It uses a common interaction model for events overlapping in neutrino energy and correlated detector s ...
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Journal ArticlePhysical Review D · December 1, 2024
A search for proton decay into e+/μ+ and a η meson has been performed using data from a 0.373 Mton·year exposure (6050.3 live days) of Super-Kamiokande. Compared to previous searches this work introduces an improved model of the intranuclear η interaction ...
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Journal ArticlePhysical Review D · October 15, 2024
We present the results of the charge ratio (R) and polarization (P0μ) measurements using decay electron events collected between September 2008 and June 2022 with the Super-Kamiokande detector. Because of its underground location and long operation, we are ...
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Journal ArticleAstrophysical Journal · October 1, 2024
Preceding a core-collapse supernova (CCSN), various processes produce an increasing amount of neutrinos of all flavors characterized by mounting energies from the interior of massive stars. Among them, the electron antineutrinos are potentially detectable ...
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Journal ArticleProgress of Theoretical and Experimental Physics · October 1, 2024
Neutrinos from very nearby supernovae, such as Betelgeuse, are expected to generate more than ten million events over 10 s in Super-Kamokande (SK). At such large event rates, the buffers of the SK analog-to-digital conversion board (QBEE) will overflow, ca ...
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ConferenceProceedings of Science · September 27, 2024
This contribution reports the results of the searches for high-energy astrophysical neutrino point sources in the energy range above GeV using Super-Kamiokande data. The searches include time-integrated and time-dependent full sky searches for both νμ ...
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ConferenceProceedings of Science · September 27, 2024
Super-Kamiokande (SK) experiment started the "SK-Gd experiment" by dissolving gadolinium (Gd) sulfate octa-hydrate in ultra-pure water from the tank in July 2020. The neutron tagging efficiency has been improved compared to the pure-water phase by detectin ...
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ConferenceProceedings of Science · September 27, 2024
Neutrinos and muons from cosmic-ray interactions in the atmosphere originate from mesons, such as pions and kaons, in air-showers. An accuracy of the absolute atmospheric neutrino flux and its flavor ratio are limited due to the uncertainty of meson produc ...
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ConferenceProceedings of Science · September 27, 2024
In 2020, a new phase of Super-Kamiokande experiment, SK-Gd, was started by loading gadolinium into the pure water. This led to a high neutron detection efficiency, which allows us to distinguish different neutrino reactions, enhance signals and remove back ...
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ConferenceProceedings of Science · September 27, 2024
The atmospheric neutrino-oxygen neutral-current quasielasatic (NCQE) reactions are one of the main background in the search for supernova relic neutrinos. Here, we report the first measurement of the atmospheric neutrino-oxygen NCQE cross section in the Su ...
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ConferenceProceedings of Science · September 27, 2024
Cosmic-ray muons are generated from the decay of mesons which are secondary particles produced via hadronic interaction between primary cosmic-ray particles and atmospheric nuclei at the upper the atmosphere. The mesons such pions and kaons mostly decay in ...
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ConferenceProceedings of Science · September 27, 2024
Super-Kamiokande is a large water Cherenkov detector located approximately 1,000 m underground in Kamioka, Japan. The detector is a cylindrical tank 39.3 m in diameter and 41.4 m high, filled with about 50 kton of gadolinium loaded water. We measured ...
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ConferenceProceedings of Science · September 27, 2024
Since 2020, Super-Kamiokande (SK) detector has been updated by loading gadolinium (Gd) as a new experimental phase, ‘SK-Gd.’ In the SK-Gd experiment, we can search low-energy electron antineutrinos via inverse-beta decay with efficient neutron identificati ...
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ConferenceProceedings of Science · September 27, 2024
Despite efforts from numerous experiments to grasp the nature of dark matter, no convincing dark matter signal has been observed so far and the very properties of this invisible matter remain unknown. Nevertheless, strong constraints on these properties ar ...
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Journal ArticleNuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment · August 1, 2024
The first loading of gadolinium (Gd) into Super-Kamiokande in 2020 was successful, and the neutron capture efficiency on Gd reached 50%. To further increase the Gd neutron capture efficiency to 75%, 26.1 tons of Gd2(SO4)3⋅8 ...
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Journal ArticlePhysical Review D · August 1, 2024
Radioactivity induced by cosmic muon spallation is a dominant source of backgrounds for O(10 MeV) neutrino interactions in water Cherenkov detectors. In particular, it is crucial to reduce backgrounds to measure the solar neutrino spectrum and find neutrin ...
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Journal ArticlePhysical Review D · August 1, 2024
The Review summarizes much of particle physics and cosmology. Using data from previous editions, plus 2,717 new measurements from 869 papers, we list, evaluate, and average measured properties of gauge bosons and the recently discovered Higgs boson, lepton ...
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Journal ArticleAstrophysical Journal · July 1, 2024
Among multimessenger observations of the next Galactic core-collapse supernova, Super-Kamiokande (SK) plays a critical role in detecting the emitted supernova neutrinos, determining the direction to the supernova (SN), and notifying the astronomical commun ...
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Journal ArticlePhysical review letters · June 2024
We report a search for time variations of the solar ^{8}B neutrino flux using 5804 live days of Super-Kamiokande data collected between May 31, 1996, and May 30, 2018. Super-Kamiokande measured the precise time of each solar neutrino interaction over 22 ca ...
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Journal ArticlePhysical Review D · May 1, 2024
An analysis of solar neutrino data from the fourth phase of Super-Kamiokande (SK-IV) from October 2008 to May 2018 is performed and the results are presented. The observation time of the dataset of SK-IV corresponds to 2970 days and the total live time for ...
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Journal ArticlePhysical Review D · April 1, 2024
We present a measurement of neutrino oscillation parameters with the Super-Kamiokande detector using atmospheric neutrinos from the complete pure-water SK I-V (April 1996-July 2020) dataset, including events from an expanded fiducial volume. The dataset co ...
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Journal ArticleMonthly Notices of the Royal Astronomical Society · March 1, 2024
One challenge for applying current weak lensing analysis tools to the Nancy Grace Roman Space Telescope is that individual images will be undersampled. Our companion paper presented an initial application of IMCOM - an algorithm that builds an optimal mapp ...
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Journal ArticleJournal of Cosmology and Astroparticle Physics · February 1, 2024
Upcoming imaging surveys will allow for high signal-to-noise measurements of galaxy clustering at small scales. In this work, we present the results of the Rubin Observatory Legacy Survey of Space and Time (LSST) bias challenge, the goal of which is to com ...
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Journal ArticleMonthly Notices of the Royal Astronomical Society · February 1, 2024
The upcoming Nancy Grace Roman Space Telescope will carry out a wide-area survey in the near-infrared. A key science objective is the measurement of cosmic structure via weak gravitational lensing. Roman data will be undersampled, which introduces new chal ...
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Journal ArticlePhysical Review D · January 1, 2024
We report the first measurement of the atmospheric neutrino-oxygen neutral-current quasielastic (NCQE) cross section in the gadolinium-loaded Super-Kamiokande (SK) water Cherenkov detector. In June 2020, SK began a new experimental phase, named SK-Gd, by l ...
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ConferenceProceedings of SPIE the International Society for Optical Engineering · January 1, 2024
The Vera C. Rubin Observatory is an integrated survey system, currently under construction in Chile, to accomplish a 10-year optical survey of the southern sky. The 8.4-meter Simonyi Survey Telescope mount is nearing completion and undergoing final verific ...
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ConferenceProceedings of SPIE the International Society for Optical Engineering · January 1, 2024
The Vera C. Rubin Observatory is nearing completion, and we are embarking on a campaign to optimize the image quality during its upcoming 10-year optical survey. Here, we present the tools and methods we are implementing to disentangle and quantify the dif ...
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Journal ArticleAstrophysical Journal Letters · July 1, 2023
We report the first search result for the flux of astrophysical electron antineutrinos for energies(10)MeV in the gadolinium-loaded Super-Kamiokande (SK) detector. In 2020 June, gadolinium was introduced to the ultrapure water of the SK detector in order t ...
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Journal ArticleMonthly Notices of the Royal Astronomical Society · June 1, 2023
We present and validate 20 deg2 of overlapping synthetic imaging surveys representing the full depth of the Nancy Grace Roman Space Telescope High-Latitude Imaging Survey (HLIS) and 5 yr of observations of the Vera C. Rubin Observatory Legacy Su ...
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Journal ArticlePhysical Review D · May 1, 2023
Cosmic-ray muons that enter the Super-Kamiokande detector cause hadronic showers due to spallation in water, producing neutrons and radioactive isotopes. These are a major background source for studies of MeV-scale neutrinos and searches for rare events. I ...
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Journal ArticleMonthly Notices of the Royal Astronomical Society · April 1, 2023
Cosmological parameter constraints from recent galaxy imaging surveys are reaching percent-level accuracy on the effective amplitude of the lensing signal, S8. The upcoming Legacy Survey of Space and Time (LSST) of the Vera C. Rubin Observatory ...
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Journal ArticlePublications of the Astronomical Society of the Pacific · March 1, 2023
The presence of fringing in astronomical Charge-Coupled Device (CCD) images will have an impact on photometric quality and measurements. Yet its impact on the Vera C. Rubin Observatory’s Legacy Survey of Space and Time (LSST) has not been fully studied. We ...
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Journal ArticlePhysical review letters · January 2023
We report a search for cosmic-ray boosted dark matter with protons using the 0.37 megaton×years data collected at Super-Kamiokande experiment during the 1996-2018 period (SKI-IV phase). We searched for an excess of proton recoils above the atmospheric neu ...
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Journal ArticleAstrophysical Journal · October 1, 2022
Super-Kamiokande has been searching for neutrino bursts characteristic of core-collapse supernovae continuously, in real time, since the start of operations in 1996. The present work focuses on detecting more distant supernovae whose event rate may be too ...
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Journal ArticleJournal of Instrumentation · October 1, 2022
We present the development of neutron-tagging techniques in Super-Kamiokande IV using a neural network analysis. The detection efficiency of neutron capture on hydrogen is estimated to be 26%, with a mis-tag rate of 0.016 per neutrino event. The uncertaint ...
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Journal ArticlePhysical Review D · October 1, 2022
We searched for proton decay via p→μ+K0 in 0.37 Mton·years of data collected between 1996 and 2018 from the Super-Kamiokande water Cherenkov experiment. The selection criteria were defined separately for KS0 and KL0 channels. No significant event excess ha ...
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Journal ArticleAstrophysical Journal · August 1, 2022
The Vera Rubin Observatory Legacy Survey of Space and Time (LSST) is expected to process ∼106 transient detections per night. For precision measurements of cosmological parameters and rates, it is critical to understand the detection efficiency, ...
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Journal ArticleAstrophysical Journal · August 1, 2022
In 2020, the Super-Kamiokande (SK) experiment moved to a new stage (SK-Gd) in which gadolinium (Gd) sulfate octahydrate was added to the water in the detector, enhancing the efficiency to detect thermal neutrons and consequently improving the sensitivity t ...
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Journal ArticleProgress of Theoretical and Experimental Physics · August 1, 2022
The Review summarizes much of particle physics and cosmology. Using data from previous editions, plus 2,143 new measurements from 709 papers, we list, evaluate, and average measured properties of gauge bosons and the recently discovered Higgs boson, lepton ...
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Journal ArticleAstroparticle Physics · June 1, 2022
Due to a very low production rate of electron anti-neutrinos (ν̄e) via nuclear fusion in the Sun, a flux of solar ν̄e is unexpected. An appearance of ν̄e in solar neutrino flux opens a new window for the new physics beyond the ...
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ConferenceProceedings of Science · March 18, 2022
Super-Kamiokande (SK) is a 50-kt water Cherenkov detector, instrumented with ∼ 13k photo-multipliers and running since 1996. It is sensitive to neutrinos with energies ranging from 4.5 MeV to several TeV. A new framework has been developed for the follow-u ...
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ConferenceProceedings of Science · March 18, 2022
The radioactivity background are among the most dangerous background for low energy neutrino analysis in Super-Kamiokande (SK), like the solar neutrino analysis. Among them, the main contribution is coming from 222Rn, which is spread in the dete ...
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ConferenceProceedings of Science · March 18, 2022
We present the results of a search for the Diffuse Supernova Neutrino Background (DSNB) at Super-Kamiokande (SK) that incorporates 22.5 × 2970 kton.days of data from its fourth data-taking phase. Two analyses, with different energy regimes covering the 9.3 ...
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Journal ArticleNuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment · March 11, 2022
In order to improve Super-Kamiokande's neutron detection efficiency and to thereby increase its sensitivity to the diffuse supernova neutrino background flux, 13 tons of Gd2(SO4)3⋅8H2O (gadolinium sulfate octahyd ...
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ConferenceProceedings of SPIE the International Society for Optical Engineering · January 1, 2022
The Rubin Observatory Commissioning Camera (ComCam) is a scaled down (144 Megapixel) version of the 3.2 Gigapixel LSSTCam which will start the Legacy Survey of Space and Time (LSST), currently scheduled to start in 2024. The purpose of the ComCam is to ver ...
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Journal ArticlePhysical Review D · December 15, 2021
We have conducted a new search for the diffuse supernova neutrino background (DSNB) flux at Super-Kamiokande (SK), with a 22.5×2970-kton·day exposure from its fourth operational phase IV. With the new analysis we improve on the existing background reductio ...
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Journal Article · December 1, 2021
The Vera Rubin Observatory Legacy Survey of Space and Time (LSST) is expected
to process ${\sim}10^6$ transient detections per night. For precision
measurements of cosmological parameters and rates, it is critical to understand
the detection efficiency, ma ...
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Journal Article · November 30, 2021
Radioactivity induced by cosmic muon spallation is a dominant source of
backgrounds for $\mathcal{O}(10)~$MeV neutrino interactions in water Cherenkov
detectors. In particular, it is crucial to reduce backgrounds to measure the
solar neutrino spectrum and ...
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Journal ArticleProgress of Theoretical and Experimental Physics · October 1, 2021
A search for neutrinos produced in coincidence with gamma-ray bursts (GRBs) was conducted with the Super-Kamiokande (SK) detector. Between December 2008 and March 2017, the Gamma-ray Coordinates Network recorded 2208 GRBs that occurred during normal SK ope ...
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Journal ArticleAstrophysical Journal · September 10, 2021
The Super-Kamiokande detector can be used to search for neutrinos in time coincidence with gravitational waves detected by the LIGO–Virgo Collaboration (LVC). Both low-energy (7–100 MeV) and high-energy (0.1–105 GeV) samples were analyzed in ord ...
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Journal ArticleAstrophysical Journal Supplement Series · March 12, 2021
Featured Publication
We describe the simulated sky survey underlying the second data challenge (DC2) carried out in preparation for analysis of the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) by the LSST Dark Energy Science Collaboration (LSST DESC). Signi ...
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Journal ArticlePhysical Review D · January 21, 2021
As a baryon number violating process with ΔB=2, neutron-antineutron oscillation (n→n¯) provides a unique test of baryon number conservation. We have performed a search for n→n¯ oscillation with bound neutrons in Super-Kamiokande, with the full dataset from ...
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Journal Article · January 12, 2021
In preparation for cosmological analyses of the Vera C. Rubin Observatory
Legacy Survey of Space and Time (LSST), the LSST Dark Energy Science
Collaboration (LSST DESC) has created a 300 deg$^2$ simulated survey as part of
an effort called Data Challenge 2 ...
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Journal Article · December 14, 2020
Due to a very low production rate of electron anti-neutrinos ($\bar{\nu}_e$)
via nuclear fusion in the Sun, we expect to see $\bar{\nu}_e$ from other
contribution. An appearance of $\bar{\nu}_e$ in solar neutrino flux opens a new
window for the new physics ...
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Journal Article · October 30, 2020
We have searched for proton decay via $p\to e^+\pi^0$ and $p\to \mu^+\pi^0$
modes with the enlarged fiducial volume data of Super-Kamiokande from April
1996 to May 2018, which corresponds to 450 kton$\cdot$years exposure. We have
accumulated about 25% more ...
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Journal Article · October 29, 2020
The commissioning team for the Vera C. Rubin observatory is planning a set of
engineering and science verification observations with the Legacy Survey of
Space and Time (LSST) commissioning camera and then the Rubin Observatory LSST
Camera. The time frame ...
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Journal ArticlePhysical Review D · October 9, 2020
We present a search for an excess of neutrino interactions due to dark matter in the form of weakly interacting massive particles (WIMPs) annihilating in the Galactic center or halo based on the data set of Super-Kamiokande-I, -II, -III and -IV taken from ...
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Journal ArticleMonthly Notices of the Royal Astronomical Society · September 1, 2020
Featured Publication
Data Challenge 1 (DC1) is the first synthetic data set produced by the Rubin Observatory Legacy Survey of Space and Time (LSST) Dark Energy Science Collaboration (DESC). DC1 is designed to develop and validate data reduction and analysis and to study the i ...
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Journal ArticleProgress of Theoretical and Experimental Physics · January 1, 2020
The Review summarizes much of particle physics and cosmology. Using data from previous editions, plus 3,324 new measurements from 878 papers, we list, evaluate, and average measured properties of gauge bosons and the recently discovered Higgs boson, lepton ...
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Journal Article · April 24, 2019
Astrophysical and cosmological observations currently provide the only
robust, empirical measurements of dark matter. Future observations with Large
Synoptic Survey Telescope (LSST) will provide necessary guidance for the
experimental dark matter program. ...
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Journal Article · March 28, 2019
Despite two decades of tremendous experimental and theoretical progress, the
riddle of the accelerated expansion of the Universe remains to be solved. On
the experimental side, our understanding of the possibilities and limitations
of the major dark energy ...
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Journal ArticleAstrophysical Journal · March 10, 2019
We describe here the most ambitious survey currently planned in the optical, the Large Synoptic Survey Telescope (LSST). The LSST design is driven by four main science themes: probing dark energy and dark matter, taking an inventory of the solar system, ex ...
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Journal Article · January 11, 2019
In this document, we present the Technical Design Report of the Upgrade of
the T2K Near Detector ND280. The goal of this upgrade is to improve the Near
Detector performance to measure the neutrino interaction rate and to constrain
the neutrino interaction ...
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Journal Article · January 6, 2019
A few times a century, a core collapse supernova (CCSN) occurs in our galaxy.
When such galactic CCSNe happen, over 99\% of its gravitational binding energy
is released in the form of neutrinos. Over a period of tens of seconds, a
powerful neutrino flux is ...
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Journal ArticlePhysical Review D · January 26, 2017
The T2K off-axis near detector, ND280, is used to make the first differential cross section measurements of muon neutrino charged current single positive pion production on a water target at energies ∼0.8 GeV. The differential measurements are presented as ...
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Journal ArticleIEEE Transactions on Applied Superconductivity · June 1, 2016
JT-60SA is a fusion experiment, which is jointly constructed by Japan and Europe and which shall contribute to the early realization of fusion energy, by providing support to the operation of ITER and by addressing key physics issues for ITER and DEMO. The ...
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ConferenceProceedings of SPIE the International Society for Optical Engineering · January 1, 2016
We employ electrostatic conversion drift calculations to match CCD pixel signal covariances observed in at field exposures acquired using candidate sensor devices for the LSST Camera.1, 2 We thus constrain pixel geometry distortions present at t ...
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Journal ArticleJournal of Instrumentation · May 1, 2015
Upcoming and current large astronomical survey experiments often seek to constrain cosmological parameters via measurements of subtle effects such as weak lensing, which can only be measured statistically. In these cases, instrumental effects in the image ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · April 10, 2015
A search for neutron-antineutron (n-n¯) oscillation was undertaken in Super-Kamiokande using the 1489 live-day or 2.45×1034 neutron-year exposure data. This process violates both baryon and baryon minus lepton numbers by an absolute value of two units and ...
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Journal ArticlePhysical review letters · September 2014
We present the results of searches for nucleon decay via n→ν[over ¯]π0 and p→ν[over ¯]π+ using data from a combined 172.8 kt·yr exposure of Super-Kamiokande-I,-II, and-III. We set lower limits on the partial lifetime for each of these modes: τn→ν[over ¯]π ...
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Journal Article · October 16, 2013
This document represents the response of the Intensity Frontier Neutrino
Working Group to the Snowmass charge. We summarize the current status of
neutrino physics and identify many exciting future opportunities for studying
the properties of neutrinos and ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · August 5, 2013
The T2K Collaboration reports evidence for electron neutrino appearance at the atmospheric mass splitting, |Δm322|≈2.4×10-3 eV2. An excess of electron neutrino interactions over background is observed from a muon neutrino beam with a peak energy ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · May 7, 2013
T2K has performed the first measurement of νμ inclusive charged current interactions on carbon at neutrino energies of ∼1 GeV where the measurement is reported as a flux-averaged double differential cross section in muon momentum and angle. The ...
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Journal ArticlePhysical review letters · May 2013
Super-Kamiokande atmospheric neutrino data were fit with an unbinned maximum likelihood method to search for the appearance of tau leptons resulting from the interactions of oscillation-generated tau neutrinos in the detector. Relative to the expectation o ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · January 2, 2013
The Tokai-to-Kamioka (T2K) experiment studies neutrino oscillations using an off-axis muon neutrino beam with a peak energy of about 0.6 GeV that originates at the Japan Proton Accelerator Research Complex accelerator facility. Interactions of the neutrino ...
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Journal ArticleProceedings, 2013 Community Summer Study on the Future of U.S. Particle Physics: Snowmass on the Mississippi (CSS2013): Minneapolis, MN, USA, July 29-August 6, 2013 · 2013Cite
ConferenceProceedings of the 33rd International Cosmic Rays Conference Icrc 2013 · January 1, 2013
Super-Kamiokande can search for dark matter by detecting neutrinos and muons which are produced by WIMP pair annihilations occur inside the Sun. The huge gravity and hydrogen-rich composition of the Sun combined with high sensitivity of Super-Kamiokande fo ...
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Journal ArticleAstroparticle Physics · August 1, 2012
GUT monopoles captured by the Sun's gravitation are expected to catalyze proton decays via the Callan-Rubakov process. In this scenario, protons, which initially decay into pions, will ultimately produce νe, νμ and ν̄ μ. Aft ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · July 23, 2012
We have searched for proton decay via p→μ +K0 using data from a 91.7kiloton•year exposure of Super-Kamiokande- I, a 49.2kiloton•year exposure of Super-Kamiokande II, and a 31.9kiloton•year exposure of Super-Kamiokande III. The number of candidat ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · June 5, 2012
Searches for a nucleon decay into a charged antilepton (e + or μ +) plus a light meson (π0, π -, η, ρ0, ρ -, ω) were performed using the Super-Kamiokande I and II data. Twelve nucleon decay modes were searched fo ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · March 22, 2012
A new Super-Kamiokande search for supernova relic neutrinos was conducted using 2853 live days of data. Sensitivity is now greatly improved compared to the 2003 Super-Kamiokande result, which placed a flux limit near many theoretical predictions. This more ...
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Journal ArticlePhysical Review D - Particles, Fields, Gravitation and Cosmology · 2012
This biennial Review summarizes much of particle physics. Using data from previous editions, plus 2658 new measurements from 644 papers, we list, evaluate, and average measured properties of gauge bosons, leptons, quarks, mesons, and baryons. We summarize ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · December 14, 2011
In this paper we study nonstandard neutrino interactions as an example of physics beyond the standard model using atmospheric neutrino data collected during the Super-Kamiokande I (1996-2001) and II (2003-2005) periods. We focus on flavor-changing-neutral- ...
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Journal ArticlePhysical review letters · December 2011
We present a search for differences in the oscillations of antineutrinos and neutrinos in the Super-Kamiokande-I, -II, and -III atmospheric neutrino sample. Under a two-flavor disappearance model with separate mixing parameters between neutrinos and antine ...
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Journal ArticleAstrophysical Journal · December 1, 2011
We present the result of an indirect search for high energy neutrinos from Weakly Interacting Massive Particle (WIMP) annihilation in the Sun using upward-going muon (upmu) events at Super-Kamiokande. Data sets from SKI-SKIII (3109.6days) were used for the ...
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Journal ArticleAip Conference Proceedings · December 1, 2011
In this talk, I explain the search for tau neutrino appearance in the atmospheric neutrino flux at Super-Kamiokande with a particular emphasis on the effect deep inelastic cross section uncertainties have on interpreting the result. In particular, I explai ...
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Journal ArticleAstronomy and Astrophysics · November 25, 2011
Aims. Over the past few years a major effort has been put into the exploration of potential sites for the deployment of submillimetre astronomical facilities. Amongst the most important sites are Dome C and Dome A on the Antarctic Plateau, and the Chajnant ...
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Journal Article · October 26, 2011
In early 2010, the Long-Baseline Neutrino Experiment (LBNE) science
collaboration initiated a study to investigate the physics potential of the
experiment with a broad set of different beam, near- and far-detector
configurations. Nine initial topics were i ...
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Journal ArticleCryogenics · July 1, 2011
The construction, commissioning, and operation phases of the W7-X cryomagnetic test facility in CEA Saclay lasted ten years. The large diversity of equipments called, specialties involved and problems solved attest the expertise that was required to operat ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · March 24, 2011
The results of the third phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first and second phase results. With improved detector calibrations, a full detector simulation, and improved analysis methods, the systemat ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · March 16, 2011
In this paper, we report on the measurement of the rate of inclusive π0 production induced by charged-current neutrino interactions in a C 8H8 target at a mean energy of 1.3 GeV in the K2K near detector. Out of a sample of 11606 charg ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · May 20, 2010
We present a search for nonzero θ13 and deviations of sin2θ23 from 0.5 in the oscillations of atmospheric neutrino data from Super-Kamiokande I, II, and III. No distortions of the neutrino flux consistent with nonzero θ13 are found and both neut ...
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Journal ArticleJournal of Physics: Conference Series · 2010
Supernova relic neutrinos (SRN) are the diffuse supernova neutrino background from all past supernovae. No experiment has succeeded in detecting SRN yet. Currently, the Super-Kamiokande experiment has the world's best flux upper limit of 1.2 e/cm2/sec for ...
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Journal ArticleJournal of High Energy Physics · December 1, 2009
In this paper, we investigate the impact in future megaton-scale water Cherenkov detectors of identifying proton Cherenkov rings. We estimate the expected event rates for detected neutral current and charged current quasi-elastic neutrino interactions from ...
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Journal ArticleAip Conference Proceedings · December 1, 2009
This is a summary of "the path forward" discussion session of the NuInt09 workshop which focused on Monte Carlo event generators. The main questions raised as part of this discussion are: how to make Monte Carlo generators more reliable and how important i ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · June 22, 2009
We report the development of a proton identification method for the Super-Kamiokande (SK) detector. This new tool is applied to the search for events with a single proton track, a high purity neutral current sample of interest for sterile neutrino searches ...
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Journal ArticlePhysical review letters · April 2009
We have searched for proton decays via p-->e;{+}pi;{0} and p-->micro;{+}pi;{0} using data from a 91.7 kt.yr exposure of Super-Kamiokande-I and a 49.2 kt.yr exposure of Super-Kamiokande-II. No candidate events were observed with expected backgrounds induced ...
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Journal ArticleAstrophysical Journal · January 1, 2009
We perform a search for neutrinos coincident with GRB 080319B - the brightest GRB observed to date - in a 1000 s window. No statistically significant coincidences were observed and we thereby obtain an upper limit on the fluence of neutrino-induced muons f ...
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Journal ArticleAstrophysical Journal · January 1, 2009
It has been hypothesized that large fluxes of neutrinos may be created in astrophysical "cosmic accelerators." The primary background for a search for astrophysical neutrinos comes from atmospheric neutrinos, which do not exhibit the pointlike directional ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · August 7, 2008
Single charged pion production in charged-current muon neutrino interactions with carbon is studied using data collected in the K2K long-baseline neutrino experiment. The mean energy of the incident muon neutrinos is 1.3 GeV. The data used in this analysis ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · February 25, 2008
The atmospheric neutrino background for proton decay via p→e+π0 in ring imaging water Cherenkov detectors is studied with an artificial accelerator neutrino beam for the first time. In total, 3.14×105 neutrino events corresponding to about 10 megaton-years ...
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Chapter · January 1, 2008
Super-Kamiokande is a 50 kiloton water Cherenkov detector located at the Kamioka Observatory of the Institute for Cosmic Ray Research, University of Tokyo. It was designed to study neutrino oscillations and carry out searches for the decay of the nucleon. ...
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Journal ArticleHippocampus · 2008
Dentate granule cells play a critical role in the function of the entorhinal-hippocampal circuitry in health and disease. Dentate granule cells are situated to regulate the flow of information into the hippocampus, a structure required for normal learning ...
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Journal ArticleEas Publications Series · August 1, 2007
The CEA, in coordination with IPEV and LUAN, will prepare an experiment to study frost formation on surfaces in radiative cooling in the winter. This experiment has been shipped to be installed at Concordia before the 2007 winter period. It will be control ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · March 23, 2007
The relative sidereal variation in the arrival direction of primary cosmic ray nuclei of median energy 10 TeV was measured using downward, through-going muons detected with the Super-Kamiokande-I detector. The projection of the anisotropy map onto the righ ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · October 20, 2006
We present measurements of νμ disappearance in K2K, the KEK to Kamioka long-baseline neutrino oscillation experiment. One-hundred and twelve beam-originated neutrino events are observed in the fiducial volume of Super-Kamiokande with an expectation of 158. ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · September 20, 2006
The weak nucleon axial-vector form factor for quasielastic interactions is determined using neutrino interaction data from the K2K Scintillating Fiber detector in the neutrino beam at KEK. More than 12000 events are analyzed, of which half are charged-curr ...
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Journal ArticlePhysical review letters · May 2006
We performed an improved search for nu(mu) --> nu(e) oscillation with the KEK to Kamioka (K2K) long-baseline neutrino oscillation experiment, using the full data sample of 9.2 x 10(19) protons on target. No evidence for a nu(e) appearance signal was found, ...
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ConferenceAnnual Meeting of the Division of Particles and Fields of the American Physical Society, DPF 2006, and the Annual Fall Meeting of the Japan Particle Physics Community · 2006
• SK-III has been started and is taking data • SK-II data has been updated to its final 791d • Oscillation analysis with SK-I, SK-II data has been performed and shows consistency with final SK-I data set • SK-II shows consistency within the global analysis ...
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ConferenceAnnual Meeting of the Division of Particles and Fields of the American Physical Society Dpf 2006 and the Annual Fall Meeting of the Japan Particle Physics Community · January 1, 2006
• SK-III has been started and is taking data • SK-II data has been updated to its final 791d • Oscillation analysis with SK-I, SK-II data has been performed and shows consistency with final SK-I data set • SK-II shows consistency within the global analysis ...
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Journal ArticleEuropean Physical Journal C · December 1, 2004
The final analysis of atmospheric neutrino events collected with the MACRO detector is presented. Three different classes of events, generated by neutrinos in different energy ranges, are studied looking at rates, angular distributions and estimated energi ...
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Journal ArticleEuropean Physical Journal C · October 1, 2004
We present the final results of the search for stellar gravitational collapses obtained by the MACRO experiment. The detector was active for a stellar collapse search for more than 11 years and it was sensitive to collapses occurring all over in our galaxy ...
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Journal ArticlePhysical review letters · September 2004
Muon neutrino disappearance probability as a function of neutrino flight length L over neutrino energy E was studied. A dip in the L/E distribution was observed in the data, as predicted from the sinusoidal flavor transition probability of neutrino oscilla ...
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Journal ArticlePhysical review letters · July 2004
A search for a nonzero neutrino magnetic moment has been conducted using 1496 live days of solar neutrino data from Super-Kamiokande-I. Specifically, we searched for distortions to the energy spectrum of recoil electrons arising from magnetic scattering du ...
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Journal ArticlePhysical review letters · July 2004
We present a search for electron neutrino appearance from accelerator-produced muon neutrinos in the K2K long-baseline neutrino experiment. One candidate event is found in the data corresponding to an exposure of 4.8 x 10(19) protons on target. The expecte ...
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Journal Article · February 2, 2004
We present the final results of a search for lightly ionizing particles using
the entire cosmic ray data set the MACRO detector collected during its
1995-2000 run. Like the original search performed with the data of 1995-96,
this search was sensitive to fr ...
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Journal ArticleAstroparticle Physics · January 1, 2004
The primary cosmic ray (CR) proton, helium and CNO fluxes in the energy range 80-300 TeV are studied at the National Gran Sasso Laboratories by means of EAS-TOP (Campo Imperatore, 2005 m a.s.l.) and MACRO (deep underground, 3100 m w.e., the surface energy ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · January 1, 2004
The time variation of the elastic scattering rate of solar neutrinos with electrons in Super-Kamiokande-I was fit to the variations expected from active two-neutrino oscillations. The best fit in the large mixing angle solution has a mixing angle of [Formu ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · January 1, 2004
We present the results of indirect searches for Weakly Interacting Massive Particles (WIMPs), with 1679.6 live days of data from the Super-Kamiokande detector using neutrino-induced upward through-going muons. The search is performed by looking for an exce ...
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Journal ArticleAstroparticle Physics · January 1, 2004
The cosmic ray primary composition in the energy range between 1015 and 1016 eV, i.e., around the "knee" of the primary spectrum, has been studied through the combined measurements of the EAS-TOP air shower array (2005 m a.s.l., 10
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Journal ArticleAstroparticle Physics · November 1, 2003
Using data collected by the MACRO experiment from 1989 to the end of its operations in 2000, we have studied in the underground muon flux the shadowing effects due to both the Moon and the Sun. We have observed the shadow cast by the Moon at its apparent p ...
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Journal ArticlePhysics Letters Section B Nuclear Elementary Particle and High Energy Physics · July 24, 2003
The energy of atmospheric neutrinos detected by MACRO was estimated using multiple Coulomb scattering of upward throughgoing muons. This analysis allows a test of atmospheric neutrino oscillations, relying on the distortion of the muon energy distribution. ...
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Journal ArticleAstroparticle Physics · June 1, 2003
The MACRO detector was located in the Hall B of the Gran Sasso underground laboratories under an average rock overburden of 3700 hg/cm2. A transition radiation detector composed of three identical modules, covering a total horizontal area of 36 ...
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Journal ArticlePhysical review letters · May 2003
We present the results of a search for low energy nu(e) from the Sun using 1496 days of data from Super-Kamiokande-I. We observe no significant excess of events and set an upper limit for the conversion probability to nu(e) of the 8B solar neutrino. This c ...
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Journal ArticleNuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment · May 1, 2003
In this talk, I will review the Super-K analysis to distinguish between the νμ→ντ oscillation hypothesis and other exotic oscillation/decay scenarios. All of the tested exotic hypotheses are excluded by the Super-K atmospheric neutrin ...
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Journal ArticleNuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment · April 1, 2003
Super-Kamiokande is the world's largest water Cherenkov detector, with net mass 50,000 tons. During the period April, 1996 to July, 2001, Super-Kamiokande I collected 1678 live-days of data, observing neutrinos from the Sun, Earth's atmosphere, and the K2K ...
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Journal ArticlePhysical review letters · February 2003
A search for the relic neutrinos from all past core-collapse supernovae was conducted using 1496 days of data from the Super-Kamiokande detector. This analysis looked for electron-type antineutrinos that had produced a positron with an energy greater than ...
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Journal ArticleNuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment · February 1, 2003
Tracking performance of the scintillating fiber detector (SciFi) in the K2K experiment was studied. SciFi was used to reconstruct charged particles produced in neutrino interactions in the near detector. The track reconstruction algorithm and the performan ...
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Journal ArticlePhysical Review D · January 1, 2003
A search for periodic modulations of the solar neutrino flux was performed using the Super-Kamiokande-I data taken from 31 May 1996 to 15 July 2001. The detector's capability of measuring the exact time of events, combined with a relatively high yield of s ...
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Journal ArticleAstroparticle Physics · January 1, 2003
The MACRO underground detector at Gran Sasso Laboratory recorded 60 million secondary cosmic ray muons from February 1989 until December 2000. Different techniques were used to analyze this sample in search for density excesses from astrophysical point-lik ...
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Journal ArticleAstroparticle Physics · January 1, 2003
Many galactic and extragalactic astrophysical sources are currently considered promising candidates as high-energy neutrino emitters. Astrophysical neutrinos can be detected as upward-going muons produced in charged-current interactions with the medium sur ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · January 1, 2003
We have analyzed 44.3M single muons collected by MACRO from 1991 through 2000 in 2145 live days of operation. We have searched for the solar diurnal, apparent sidereal, and pseudosidereal modulation of the underground muon rate by computing hourly deviatio ...
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Journal ArticlePhysical review letters · January 2003
The K2K experiment observes indications of neutrino oscillation: a reduction of nu(mu) flux together with a distortion of the energy spectrum. Fifty-six beam neutrino events are observed in Super-Kamiokande (SK), 250 km from the neutrino production point, ...
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Journal ArticleNuclear Physics B Proceedings Supplements · January 1, 2003
We present the final results of the search for exotic massive particles in the cosmic radiation performed with the MACRO underground experiment. Magnetic monopoles and nuclearites flux upper limits obtained with the CR39 nuclear track subdetector, the scin ...
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Journal ArticlePhysical Review Letters · 2003
A study was performed on Kamioka long-baseline neutrino oscillation experiment (K2K). The indications of neutrino oscillation such as a reduction of flux together with a distortion of the energy spectrum were observed in the experiment. In Super Kamiokande ...
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Journal ArticleNuclear Physics B Proceedings Supplements · January 1, 2003
The K2K experiment has collected approximately half of its allocated protons on target between June of 1999 and July of 2001. These proceedings give a short introduction to the experiment and summarize some of the recent results. ...
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Journal ArticleEuropean Physical Journal C · December 1, 2002
The interaction of a Grand Unification Magnetic Monopole with a nucleon can lead to a barion-number violating process in which the nucleon decays into a lepton and one or more mesons (catalysis of nucleon decay). In this paper we report an experimental stu ...
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Journal ArticleEuropean Physical Journal C · November 1, 2002
We present the final results obtained by the MACRO experiment in the search for GUT magnetic monopoles in the penetrating cosmic radiation, for the range 4 × 10-5 < β < 1. Several searches with all the MACRO sub-detectors (i.e. scintillation cou ...
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Journal ArticleNuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment · October 21, 2002
Muon energy measurement represents an important issue for any experiment addressing neutrino-induced up-going muon studies. Since the neutrino oscillation probability depends on the neutrino energy, a measurement of the muon energy adds an important piece ...
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Journal ArticleAstrophysical Journal · October 10, 2002
Using the Super-Kamiokande neutrino observatory, a search was conducted for neutrinos produced in coincidence with gamma-ray bursts observed by the Burst and Transient Source Experiment detector. Super-Kamiokande data in the neutrino energy range of 7 MeV ...
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Journal Article · October 2, 2002
The NuMI neutrino beam line and the MINOS experiment represent a major
investment of US High Energy Physics in the area of neutrino physics. The
forthcoming results could decisively establish neutrino oscillations as the
underlying physics mechanism for th ...
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Journal ArticlePhysics Letters Section B Nuclear Elementary Particle and High Energy Physics · July 18, 2002
A number of different fits to solar neutrino mixing and mass square difference were performed using 1496 days of Super-Kamiokande-I's solar neutrino data. These data select two allowed areas at large neutrino mixing when combined with either the solar
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Journal ArticleAstroparticle Physics · July 8, 2002
We describe a search method for fast moving (β = v/c > 5 × 10-3) magnetic monopoles using simultaneously the scintillator, streamer tube and track-etch subdetectors of the MACRO apparatus. The first two subdetectors are used primarily for the id ...
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Journal ArticleNuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment · July 1, 2002
MACRO was an experiment that ran in the Laboratori Nazionali del Gran Sasso from 1988 to 2000. Its principal goal was to observe magnetic monopoles or set significantly lower experimental flux limits than had been previously available in the velocity range ...
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Journal Article · June 12, 2002
In this 2001 status report of the MACRO experiment, results are presented on
atmospheric neutrinos and neutrino oscillations, high energy neutrino
astronomy, searches for WIMPs, search for low energy stellar gravitational
collapse neutrinos, stringent uppe ...
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Journal ArticleNuclear Physics B Proceedings Supplements · January 1, 2002
The near detector complex of the K2K long-baseline neutrino experiment contains a scintillating fiber tracking detector. It is capable of detecting not only the muon but also the outgoing proton in neutrino-nucleon scattering. This allows for the enhanceme ...
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Journal ArticlePhysics Letters Section B Nuclear Elementary Particle and High Energy Physics · September 27, 2001
The angular distribution of upward-going muons produced by atmospheric neutrinos in the rock below the MACRO detector shows anomalies in good agreement with two flavor vμ → vτ oscillations with maximum mixing and Δm2 around ...
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Journal ArticlePhysics Letters Section B Nuclear Elementary Particle and High Energy Physics · July 5, 2001
The KEK to Kamioka long-baseline neutrino experiment (K2K) has begun its investigation of neutrino oscillations suggested by atmospheric neutrino observations. Twenty-eight neutrino events have been detected in coincidence with the expected arrival time of ...
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Journal ArticlePhysical review letters · June 2001
Solar neutrino measurements from 1258 days of data from the Super-Kamiokande detector are presented. The measurements are based on recoil electrons in the energy range 5.0-20.0 MeV. The measured solar neutrino flux is 2.32+/-0.03(stat)+0.08-0.07(syst)x10(6 ...
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Journal ArticlePhysical review letters · June 2001
We report the result of a search for neutrino oscillations using precise measurements of the recoil electron energy spectrum and zenith angle variations of the solar neutrino flux from 1258 days of neutrino-electron scattering data in Super-Kamiokande. The ...
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Journal ArticlePlant physiology · April 2001
The metabolism of polyamines (putrescine, spermidine, and spermine) has become the target of genetic manipulation because of their significance in plant development and possibly stress tolerance. We studied the polyamine metabolism in non-transgenic (NT) a ...
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Journal ArticleNUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT · February 11, 2001Link to itemCite
Journal ArticleAstrophysical Journal · January 10, 2001
High-energy gamma-ray astronomy is now a well-established field, and several sources have been discovered in the region from a few giga-electron volts up to several tera-electron volts. If sources involving hadronic processes exist, the production of photo ...
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Journal ArticleNuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment · 2001
The decay of 16N is used to cross check the absolute energy scale calibration for solar neutrinos established by the electron linear accelerator (LINAC). A deuterium-tritium neutron generator was employed to create 16N via the (n,p) reaction on 16O in the ...
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Journal ArticlePhysical Review D · December 1, 2000
A search for lightly ionizing particles has been performed with the MACRO detector. This search was sensitive to particles with charges between 1/5 e and close to the charge of an electron, with β between approximately 0.25 and 1.0. Unlike previous searche ...
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Journal ArticlePhysical review letters · November 2000
The previously published atmospheric neutrino data did not distinguish whether muon neutrinos were oscillating into tau neutrinos or sterile neutrinos, as both hypotheses fit the data. Using data recorded in 1100 live days of the Super-Kamiokande detector, ...
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Journal ArticleNuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment · October 11, 2000
We describe the construction and performance of a scintillating fiber detector used in the near detector for the K2K (KEK to Kamioka, KEK E362) long baseline neutrino oscillation experiment. The detector uses 3.7 m long and 0.692 mm diameter scintillating ...
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Journal ArticleNuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment · July 21, 2000
A new combined test of an electromagnetic liquid argon accordion calorimeter and a hadronic scintillating-tile calorimeter was carried out at the CERN SPS. These devices are prototypes of the barrel calorimeter of the future ATLAS experiment at the LHC. Th ...
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Journal ArticlePhysics Letters Section B Nuclear Elementary Particle and High Energy Physics · April 6, 2000
We present the measurement of two event samples induced by atmospheric v(μ) of average energy Ē(ν) ~ 4 GeV. In the first sample, a neutrino interacts inside the MACRO detector producing an upward-going muon leaving the apparatus. The ratio of the number of ...
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Journal ArticlePhysical Review D - Particles, Fields, Gravitation and Cosmology · 2000
A search for lightly ionizing particles has been performed with the MACRO detector. This search was sensitive to particles with charges between 1/5 e and close to the charge of an electron, with β between approximately 0.25 and 1.0. Unlike previous searche ...
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Journal ArticleNuclear Physics B Proceedings Supplements · January 1, 2000
Searches for massive penetrating particles in the cosmic radiation have been performed with the MACRO detector. Scintillators, streamer tubes (instrumented with specialized electronics) and nuclear track detectors have been used to search for signatures co ...
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Journal ArticleNuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment · January 21, 1999
In order to calibrate the Super-Kamiokande experiment for solar neutrino measurements, a linear accelerator (LINAC) for electrons was installed at the detector. LINAC data were taken at various positions in the detector volume, tracking the detector respon ...
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Journal ArticleNuclear Physics B Proceedings Supplements · January 1, 1999
With the aim of discussing the effect of the possible sources of systematic uncertainties in simulation models, the analysis of multiple muon events from the MACRO experiment at Gran Sasso is reviewed. In particular, the predictions from different currentl ...
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Journal ArticlePhysics Letters Section B Nuclear Elementary Particle and High Energy Physics · January 1, 1999
A total of 137 upward stopping muons of minimum energy 1.6 GeV are observed by Super-Kamiokande during 516 detector live days. The measured muon flux is 0.39 ± 0.04(stat.) ± 0.02(syst.) × 10-13 cm-2s-1sr-1 compar ...
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Journal ArticlePhysical Review Letters · January 1, 1999
We present results of a search for proton decays, p → ¯νK+, using data from a 33kt?yr exposure of the Super-Kamiokande detector. Two decay modes of the kaon, K+ → µ+νµ and K+ → π+π0
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Journal ArticlePhysical Review Letters · January 1, 1999
A search for day-night variations in the solar neutrino flux resulting from neutrino oscillations has been carried out using the 504 day sample of solar neutrino data obtained at Super-Kamiokande. The absence of a significant day-night variation has set an ...
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Journal ArticlePhysical Review Letters · January 1, 1999
A measurement of the energy spectrum of recoil electrons from solar neutrino scattering in the Super-Kamiokande detector is presented. The results shown here were obtained from 504 days of data taken between 31 May 1996 and 25 March 1998. The shape of the ...
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Journal ArticlePhysics Letters Section B Nuclear Elementary Particle and High Energy Physics · January 1, 1999
Radioactivity from radon is a major background for observing solar neutrinos at Super-Kamiokande. In this paper, we describe the measurement of radon concentrations at Super-Kamiokande, the method of radon reduction, and the radon monitoring system. The me ...
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Journal ArticlePhysical Review Letters · January 1, 1999
A total of 614 upward throughgoing muons of minimum energy 1.6 GeV are observed by Super-Kamiokande during 537 detector live days. The measured muon flux is [1.74±0.07(stat)±0.02(sys)]×10-13cm-2s-1sr-1 compared t ...
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Journal ArticleAstroparticle Physics · January 1, 1999
We have measured directly the residual energy of cosmic ray muons crossing the MACRO detector at the Gran Sasso Laboratory. For this measurement we have used a transition radiation detector consisting of three identical modules, each of about 12m2
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · January 1, 1999
We perform an indirect search for weakly interacting massive particles (WIMPs) using the MACRO detector to look for neutrino-induced upward-going muons resulting from the annihilation of WIMPs trapped in the Sun and Earth. The search is conducted in variou ...
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Journal ArticlePhysical Review Letters · January 1, 1999
The east-west anisotropy, caused by the deflection of primary cosmic rays in the Earth's magnetic field, is observed for the first time in the flux of atmospheric neutrinos. Using a 45 kt yr exposure of the Super-Kamiokande detector, 552 e-like and 633 μ-l ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · January 1, 1999
We present a measurement of the underground decoherence function using multi-muon events observed in the MACRO detector at Gran Sasso at an average depth of (Formula presented) Muon pair separations up to 70 m have been measured, corresponding to parent me ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · January 1, 1999
Using data collected by the MACRO experiment during the years 1989–1996, we show evidence for the shadow of the Moon in the underground cosmic ray flux with a significance of 3.6σ. This detection of the shadowing effect is the first by an underground detec ...
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Journal ArticlePhysics Letters Section B Nuclear Elementary Particle and High Energy Physics · September 17, 1998
The flavor ratio of the atmospheric neutrino flux and its zenith angle dependence have been studied in the multi-GeV energy range using an exposure of 25.5 kiloton-years of the Super-Kamiokande detector. By comparing the data to a detailed Monte Carlo simu ...
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Journal ArticlePhysics Letters Section B Nuclear Elementary Particle and High Energy Physics · August 27, 1998
We present a measurement of the flux of neutrino-induced upgoing muons (< Eν > ∼ 100 GeV) using the MACRO detector. The ratio of the number of observed to expected events integrated over all zenith angles is 0.74 ± 0.036 (stat) ± 0.046 (systemat ...
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Journal ArticlePhysics Letters Section B Nuclear Elementary Particle and High Energy Physics · August 6, 1998
From an exposure of 25.5 kiloton-years of the Super-Kamiokande detector, 900 muon-like and 983 electron-like single-ring atmospheric neutrino interactions were detected with momentum pe > 100 MeV/c, pμ > 200 MeV/c, and with visible en ...
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Journal ArticleNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment · July 1998Full textCite
Journal ArticlePhysical Review Letters · January 1, 1998
The first results of the solar neutrino flux measurement from Super-Kamiokande are presented. The results shown here are obtained from data taken between 31 May 1996, and 23 June 1997. Using our measurement of recoil electrons with energies above 6.5 MeV, ...
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Journal ArticlePhysical Review Letters · January 1, 1998
We present an analysis of atmospheric neutrino data from a 33.0 kton yr (535-day) exposure of the Super-Kamiokande detector. The data exhibit a zenith angle dependent deficit of muon neutrinos which is inconsistent with expectations based on calculations o ...
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Journal ArticleAstroparticle Physics · January 1, 1998
An experimental study of the production of up-going charged particles in inelastic interactions of down-going underground muons is reported, using data obtained from the MACRO detector at the Gran Sasso Laboratory. In a sample of 12.2 x 106 sing ...
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Journal ArticleAstroparticle Physics · January 1, 1998
The MACRO experiment has been running as a supernova neutrino detector since 1989 and is sensitive to the whole galaxy since the beginning of 1992. A galactic supernova would produce some hundreds of v̄e events in the detector. We describe our st ...
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Journal ArticlePhysical Review Letters · January 1, 1998
We have searched for proton decay via p→e+π0 using data from a 25.5ktonyr exposure of the Super-Kamiokande detector. We find no candidate events with an expected background induced by atmospheric neutrinos of 0.1 events. From these da ...
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Journal ArticlePhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics · 1998
From an exposure of 25.5 kiloton-years of the Super-Kamiokande detector, 900 muon-like and 983 electron-like single-ring atmospheric neutrino interactions were detected with momentum pe > 100 MeV/c, pμ > 200 MeV/c, and with visible energy less than 1 ...
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Journal ArticleNuclear Physics B Proceedings Supplements · January 1, 1998
The MACRO underground detector at Gran Sasso has recorded about 30 million muon events in the period 1989-1995. We have analyzed these data to look for time variations and to study the pointing capabilities of the apparatus in the search for astrophysical ...
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Journal ArticlePhysics Letters Section B Nuclear Elementary Particle and High Energy Physics · August 7, 1997
In this letter we present the results of the search for massive magnetic monopoles in the penetrating cosmic ray radiation using the various subdetectors of the MACRO apparatus, during the period 1989-1995. Flux limits are given for the β = v/c range 4 × 1 ...
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Journal ArticleAstroparticle Physics · January 1, 1997
Using 5.33 × 106 single muons collected in 1.46 × 104 live hours by MACRO during the period 1991-1994, we have searched for a correlation between variations in the underground muon rate, Νμ, and seasonal temperature variati ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · January 1, 1997
In this paper, the first of a two-part work, we present the reconstruction and measurement of muon events detected underground by the MACRO experiment at Gran Sasso [Formula presented] 1.3 TeV in atmosphere). The main aim of this work is to discuss the muo ...
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Journal ArticlePhysical Review D Particles Fields Gravitation and Cosmology · January 1, 1997
Multimuon data from the MACRO experiment at Gran Sasso have been analyzed using a new method, which allows one to estimate the primary cosmic ray fluxes. The estimated all-particle spectrum is higher and flatter than the one obtained from direct measuremen ...
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Journal ArticlePhysics Letters B · September 7, 1995
We report on the first measurement of the flux of upgoing muons resulting from interactions of atmospheric neutrinos in the rock below MACRO. The ratio of the observed to the expected number of events integrated over all nadir angles is 0.73 ± .09stat ...
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Journal ArticleAstroparticle Physics · January 1, 1995
We describe the techniques chosen to search tor magnetic monopoles using the MACRO streamer tube sub-system. The hardware and the details of the analysis procedures will be discussed also. The results for slowly moving monopoles are reported from a first d ...
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Journal ArticlePhysics Letters B · October 13, 1994
A study of the primary cosmic ray composition in the energy range 5ṡ1014-5ṡ1015 eV is performed through the analysis of the deep underground muons and of the e.m. component of Extensive Air Showers detected in coincidence by the MACRO ...
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Journal Article · October 3, 1994
The MACRO experiment at Gran Sasso provides means for detailed studies of
multiple coincident penetrating cosmic ray muons. In this paper we concentrate
on the studies of the ultrahigh energy primary cosmic ray composition using
muon bundle multiplicities, ...
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Journal ArticleNuclear Physics B Proceedings Supplements · January 1, 1994
Muon events collected with the streamer tube system of MACRO have been used to study the vertical muon intensity and to search for astrophysical point sources. New upper limits on the muon fluxes coming from source candidates have been obtained. The μ pair ...
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Journal ArticleNuclear Physics Section B · February 17, 1992
We present a study of the correlations in the arrival times of about 1016 single and multiple muons detected by the first two MACRO supermodules. The time correlations, from milliseconds to several hundrends of seconds, have been analyzed in ter ...
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Journal ArticleNuclear Physics B Proceedings Supplements · January 1, 1992
The simultaneous observation of the electromagnetic and TeV muon components of extensive air showers by the EAS-TOP and MACRO detectors, respectively, is described for a period of 100 days in 1990. The two detectors and their combined resolutions are brief ...
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Journal ArticleNuclear Physics B Proceedings Supplements · January 1, 1992
The first MACRO lower supermodule has been sensitive to antineutrinos from stellar gravitational collapse since spring 1989. The results with the 44 tonnes of liquid scintillator which have been instrumented to search for stellar gravitational collapse are ...
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Journal ArticleNuclear Physics B Proceedings Supplements · January 1, 1991
The MACRO detector is sensitive to any fast or slow highly ionizing massive particles in cosmic rays. These include "nuclearites" or strange quark matter. The negative result of a search lasting about 20 months using 1 12 of the detector has yielded a flux ...
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